{ "id": "1004.2368", "version": "v1", "published": "2010-04-14T10:44:59.000Z", "updated": "2010-04-14T10:44:59.000Z", "title": "Statistical Analysis of Water Masers in Star-Forming Regions: Cepheus A and W75 N", "authors": [ "L. Uscanga", "J. Cantó", "J. F. Gómez", "G. Anglada", "J. M. Torrelles", "N. A. Patel", "A. C. Raga", "S. Curiel" ], "comment": "16 pages, 8 figures, and 3 tables. Accepted by The Astrophysical Journal", "categories": [ "astro-ph.GA", "astro-ph.SR" ], "abstract": "We have done a statistical analysis of Very Long Baseline Array (VLBA) data of water masers in the star-forming regions (SFRs) Cepheus A and W75 N, using correlation functions to study the spatial clustering and Doppler-velocity distribution of these masers. Two-point spatial correlation functions show a characteristic scale size for clusters of water maser spots < or ~1 AU, similar to the values found in other SFRs. This suggests that the scale for water maser excitation tends to be < or ~1 AU. Velocity correlation functions show power-law dependences with indices that can be explained by regular velocity fields, such as expansion and/or rotation. These velocity fields are similar to those indicated by the water maser proper-motion measurements; therefore, the velocity correlation functions appear to reveal the organized motion of water maser spots on scales larger than 1 AU.", "revisions": [ { "version": "v1", "updated": "2010-04-14T10:44:59.000Z" } ], "analyses": { "keywords": [ "statistical analysis", "star-forming regions", "water maser spots", "two-point spatial correlation functions", "water maser proper-motion measurements" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/715/1/132", "journal": "The Astrophysical Journal", "year": 2010, "month": "May", "volume": 715, "number": 1, "pages": 132 }, "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable", "inspire": 851939, "adsabs": "2010ApJ...715..132U" } } }